Zobrazeno 1 - 10
of 573
pro vyhledávání: '"Rol, E"'
Autor:
Mong, Y. -L., Ackley, K., Killestein, T. L., Galloway, D. K., Dyer, M., Cutter, R., Brown, M. J. I., Lyman, J., Ulaczyk, K., Steeghs, D., Dhillon, V., O'Brien, P., Ramsay, G., Noysena, K., Kotak, R., Breton, R., Nuttall, L., Palle, E., Pollacco, D., Thrane, E., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B. P., Heikkila, T., Irawati, P., Kennedy, M., Levan, A., Littlefair, S., Makrygianni, L., Marsh, T., Sanchez, D. Mata, Mattila, S., Maund, J. R., McCormac, J., Mkrtichian, D., Mullaney, J., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strom, P., Tooke, S., Wiersema, K.
Developing an effective automatic classifier to separate genuine sources from artifacts is essential for transient follow-ups in wide-field optical surveys. The identification of transient detections from the subtraction artifacts after the image dif
Externí odkaz:
http://arxiv.org/abs/2209.06375
Autor:
Steeghs, D., Galloway, D. K., Ackley, K., Dyer, M. J., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. L., Dhillon, V., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L. K., Palle, E., Breton, R. P., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkila, T., Irawati, P., Kennedy, M. R., Killestein, T., Kuncarayakti, H., Levan, A. J., Littlefair, S., Makrygianni, L., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mullaney, J., Noysena, K., Patel, M., Rol, E., Sawangwit, U., Stanway, E. R., Starling, R., Strom, P., Tooke, S., West, R., White, D. J., Wiersema, K.
The Gravitational-wave Optical Transient Observer (GOTO) is an array of wide-field optical telescopes, designed to exploit new discoveries from the next generation of gravitational wave detectors (LIGO, Virgo, KAGRA), study rapidly evolving transient
Externí odkaz:
http://arxiv.org/abs/2110.05539
Autor:
Mong, Y. -L., Ackley, K., Galloway, D. K., Dyer, M., Cutter, R., Brown, M. J. I., Lyman, J., Ulaczyk, K., Steeghs, D., Dhillon, V., OBrien, P., Ramsay, G., Noysena, K., Kotak, R., Breton, R., Nuttall, L., Palle, E., Pollacco, D., Thrane, E., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkila, T., Irawati, P., Kennedy, M., Killestein, T., Levan, A., Littlefair, S., Makrygianni, L., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mullaney, J., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strom, P., Tooke, S., Wiersema, K.
The typical detection rate of $\sim1$ gamma-ray burst (GRB) per day by the \emph{Fermi} Gamma-ray Burst Monitor (GBM) provides a valuable opportunity to further our understanding of GRB physics. However, the large uncertainty of the \emph{Fermi} loca
Externí odkaz:
http://arxiv.org/abs/2108.11802
Autor:
Makrygianni, L., Mullaney, J., Dhillon, V., Littlefair, S., Ackley, K., Dyer, M. J., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. -L., Steeghs, D., Galloway, D. K., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Breton, R., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M., Killestein, T., Levan, A., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strøm, P. A., Tooke, S., Wiersema, K.
We have adapted the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Science Pipelines to process data from the Gravitational-Wave Optical Transient Observer (GOTO) prototype. In this paper, we describe how we used the Rubin Observato
Externí odkaz:
http://arxiv.org/abs/2105.05128
Autor:
Killestein, T. L., Lyman, J., Steeghs, D., Ackley, K., Dyer, M. J., Ulaczyk, K., Cutter, R., Mong, Y. -L., Galloway, D. K., Dhillon, V., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Breton, R. P., Nuttall, L. K., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M. R., Levan, A., Littlefair, S., Makrygianni, L., Sánchez, D. Mata, Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mullaney, J., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Strøm, P. A., Tooke, S., Wiersema, K., Williams, S. C.
Large-scale sky surveys have played a transformative role in our understanding of astrophysical transients, only made possible by increasingly powerful machine learning-based filtering to accurately sift through the vast quantities of incoming data g
Externí odkaz:
http://arxiv.org/abs/2102.09892
Autor:
Mullaney, J. R., Makrygianni, L., Dhillon, V., Littlefair, S., Ackley, K., Dyer, M., Lyman, J., Ulaczyk, K., Cutter, R., Mong, Y. L., Steeghs, D., Galloway, D. K., O'Brien, P., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Breton, R., Burhanudin, U., Chote, P., Chrimes, A., Daw, E., Duffy, C., Eyles-Ferris, R., Gompertz, B., Heikkilä, T., Irawati, P., Kennedy, M., Killestein, T., Levan, A., Marsh, T., Mata-Sanchez, D., Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Rol, E., Sawangwit, U., Stanway, E., Starling, R., Tooke, S., Wiersema, K.
The past few decades have seen the burgeoning of wide field, high cadence surveys, the most formidable of which will be the Legacy Survey of Space and Time (LSST) to be conducted by the Vera C. Rubin Observatory. So new is the field of systematic tim
Externí odkaz:
http://arxiv.org/abs/2010.15142
Autor:
Gompertz, B. P., Cutter, R., Steeghs, D., Galloway, D. K., Lyman, J., Ulaczyk, K., Dyer, M. J., Ackley, K., Dhillon, V. S., O'Brien, P. T., Ramsay, G., Poshyachinda, S., Kotak, R., Nuttall, L., Breton, R. P., Pallé, E., Pollacco, D., Thrane, E., Aukkaravittayapun, S., Awiphan, S., Brown, M. J. I., Burhanudin, U., Chote, P., Chrimes, A. A., Daw, E., Duffy, C., Eyles-Ferris, R. A. J., Heikkilä, T., Irawati, P., Kennedy, M. R., Killestein, T., Levan, A. J., Littlefair, S., Makrygianni, L., Marsh, T., Sánchez, D. Mata, Mattila, S., Maund, J., McCormac, J., Mkrtichian, D., Mong, Y. -L., Mullaney, J., Müller, B., Obradovic, A., Rol, E., Sawangwit, U., Stanway, E. R., Starling, R. L. C., Strøm, P., Tooke, S., West, R., Wiersema, K.
We report the results of optical follow-up observations of 29 gravitational-wave triggers during the first half of the LIGO-Virgo Collaboration (LVC) O3 run with the Gravitational-wave Optical Transient Observer (GOTO) in its prototype 4-telescope co
Externí odkaz:
http://arxiv.org/abs/2004.00025
Autor:
Borisov, G., Devogèle, M., Cellino, A., Bagnulo, S., Christou, A., Bendjoya, Ph., Rivet, J. -P., Abe, L., Vernet, D., Donchev, Z., Krugly, Yu., Belskaya, I., Bonev, T., Steeghs, D., Galloway, D., Dhillon, V., O'Brien, P., Pollacco, D., Poshyachinda, S., Ramsay, G., Thrane, E., Ackley, K., Rol, E., Ulaczyk, K., Cutter, R., Dyer, M.
Asteroid (3200) Phaethon is a Near-Earth Apollo asteroid with an unusual orbit that brings it closer to the Sun than any other known asteroid. Its last close approach to the Earth was in mid-December 2017 and the next one will be on October 2026. Pre
Externí odkaz:
http://arxiv.org/abs/1807.11842
Autor:
Postigo, A. de Ugarte, Thoene, C. C., Bensch, K., van der Horst, A. J., Kann, D. A., Cano, Z., Izzo, L., Goldoni, P., Martin, S., Filgas, R., Schady, P., Gorosabel, J., Bikmaev, I., Bremer, M., Burenin, R., Castro-Tirado, A. J., Covino, S., Fynbo, J. P. U., Garcia-Appadoo, D., de Gregorio-Monsalvo, I., Jelinek, M., Khamitov, I., Kamble, A., Kouveliotou, C., Kruehler, T., Melnikov, S., Nardini, M., Perley, D. A., Petitpas, G., Pooley, G., Rau, A., Rol, E., Sanchez-Ramirez, R., Starling, R. L. C., Tanvir, N. R., Wiersema, K., Wijers, R. A. M. J., Zafar, T.
Publikováno v:
A&A 620, A190 (2018)
Long gamma-ray bursts give us the chance to study both their extreme physics and the star-forming galaxies in which they form. GRB 100418A, at a z = 0.6239, had a bright optical and radio afterglow, and a luminous star-forming host galaxy. This allow
Externí odkaz:
http://arxiv.org/abs/1807.04281
Autor:
Carbone, D., Garsden, H., Spreeuw, H., Swinbank, J. D., van der Horst, A. J., Rowlinson, A., Broderick, J. W., Rol, E., Law, C., Molenaar, G., Wijers, R. A. M. J.
PySE is a Python software package for finding and measuring sources in radio telescope images. The software was designed to detect sources in the LOFAR telescope images, but can be used with images from other radio telescopes as well. We introduce th
Externí odkaz:
http://arxiv.org/abs/1802.09604